We assess the age of nine planet-bearing (PB) F stars by comparing their me
tallicity, Hp variability, brightness anomaly, and location in the color-ma
gnitude diagram with the same parameters for the Hyades and field F stars.
Combined evidence from these parameters suggests that the age of our PB F s
tars is not very much different from the age of the Hyades, similar to 700
Myr, and is much younger than the ages of cooler, solar-type PB stars found
in a number of recent studies.